5XMM J182629.4-133734
5XMM-DR15 stacked source · SRCID 3005454050100019
Position:
18h26m29.41s -13d37m34.2s
(276.62256°, -13.62617°)
EP flux
1.31e-14
± 5.5e-15
erg cm-2 s-1
CLASSX
Gal_XRB
(0.485)
Detections
2
| SRCID | 3005454050100019 |
|---|---|
| IAUNAME | 5XMM J182629.4-133734 |
| SC_RA | 18h26m29.41s (276.62256°) |
| SC_DEC | -13d37m34.2s (-13.62617°) |
| RADEC_ERR | 1.24 arcsec |
| LII / BII | 17.9902° / -0.7710° |
| N_CONTRIB | 2 (detections) |
| N_OBS | 2 (observations covering the position) |
| MJD_FIRST | 52198.198 (2001-10-16 04:44:36.000 UTC) |
| MJD_LAST | 52200.500 (2001-10-18 11:59:36.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.31e-14 ± 5.5e-15 erg cm-2 s-1
Hardness ratios
HR1
1.00
± 0.35
0.2-0.5 / 0.5-1.0 keV
HR2
0.69
± 0.18
0.5-1.0 / 1.0-2.0 keV
HR3
-0.26
± 0.18
1.0-2.0 / 2.0-4.5 keV
HR4
-0.78
± 0.29
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -1.4)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Gal_XRB
CLASSX outlier: 4.77
Class probabilities
Class taxonomy
- AGN — active galactic nucleus.
- Bkg_AGN — background AGN.
- Star — Galactic star.
- Gal_XRB — Galactic X-ray binary.
- Extragal_XRB — extragalactic X-ray binary.
- CV — cataclysmic variable.
- Extended — cluster or galaxy.
Optical Monitor (OM)
- OM Source ID
- 5391767
- Match probability
- 0.671
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | — | — |
| B | — | — |
| V | 17.015 | 0.029 |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.22e-14 (+2.0e-14 / −6.2e-15) erg cm−2 s−1 |
|---|---|
| NH | 2.52e+21 (+7.3e+21 / −1.3e+20) cm−2 |
| Photon index (Γ) | 2.00 (+2.69 / −1.36) |
| DoF | 54 |
| p-value | 0.359 |
| Quality flag | 0 |
No variability data available for this source.
No contributing observations found.
Sky view (optical)
DSS2 colour optical image. The header thumbnail shows the XMM-Newton X-ray image; use the layers menu in the toolbar to switch surveys.
Hardness-ratio diagram
No hardness-ratio pairs available for this source.
The per-observation light curve is shown in the X-ray properties section above.